UV Luminosity Functions atz∼4, 5, and 6 from the Hubble Ultra Deep Field and Other DeepHubble Space TelescopeACS Fields: Evolution and Star Formation History-Reference-Cited by-同舟云学术

UV Luminosity Functions atz∼4, 5, and 6 from the Hubble Ultra Deep Field and Other DeepHubble Space TelescopeACS Fields: Evolution and Star Formation History

Published:2007-12 Issue:2 Volume:670 Page:928-958
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Bouwens R. J.,Illingworth G. D.,Franx Marijn,Ford Holland

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference136 articles.

1. Multiwavelength Observations of Dusty Star Formation at Low and High Redshift

2. The GALEX VIMOS-VLT Deep Survey Measurement of the Evolution of the 1500 Å Luminosity Function

3. Evidence for Reionization at [ITAL][CLC]z[/CLC][/ITAL] ∼ 6: Detection of a Gunn-Peterson Trough in a [ITAL][CLC]z[/CLC][/ITAL] = 6.28 Quasar

4. The Hubble Ultra Deep Field

5. The Distribution of High‐Redshift Galaxy Colors: Line‐of‐Sight Variations in Neutral Hydrogen Absorption

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